Table A.1.
Controlled sample
| planet | P[day] | M[MEarth] | R[REarth] | ρrel | ΔMMR | method | source |
|---|---|---|---|---|---|---|---|
| TOI-178 g | 20.717 | 4.40 ± 0.38 | 2.939 ± 0.056 | 0.421 ± 0.038 | 0.001 | TTV | (Leleu et al. 2024) |
| K2-138 e | 8.261 | 12.97 ± 1.99 | 3.39 ± 0.13 | 1.00 ± 0.16 | 0.001 | RV | (Lopez et al. 2019) |
| K2-138 f | 12.758 | 1.63 ± 1.65 | 2.90 ± 0.14 | 0.16 ± 0.16 | 0.001 | RV | (Lopez et al. 2019) |
| Kepler-223 b | 7.385 | 7.40 ± 1.20 | 2.99 ± 0.23 | 0.69 ± 0.14 | 0.001 | TTV | (Mills et al. 2016) |
| Kepler-223 c | 9.848 | 5.10 ± 1.40 | 3.44 ± 0.25 | 0.39 ± 0.11 | 0.001 | TTV | (Mills et al. 2016) |
| Kepler-26 c | 17.250 | 7.48 ± 0.48 | 3.11 ± 0.14 | 0.658 ± 0.062 | 0.006 | TTV | (Leleu et al. 2023) |
| Kepler-26 b | 12.280 | 4.85 ± 0.43 | 3.22 ± 0.15 | 0.406 ± 0.045 | 0.006 | TTV | (Leleu et al. 2023) |
| Kepler-177 b | 36.855 | 5.84 ± 0.84 | 3.50 ± 0.17 | 0.430 ± 0.069 | 0.007 | TTV | (Vissapragada et al. 2020) |
| K2-266 e | 19.482 | 14.30 ± 5.70 | 2.73 ± 0.12 | 1.53 ± 0.62 | 0.008 | TTV | (Rodriguez et al. 2018) |
| K2-266 d | 14.697 | 8.90 ± 4.75 | 2.93 ± 0.13 | 0.86 ± 0.46 | 0.008 | TTV | (Rodriguez et al. 2018) |
| Kepler-11 d | 22.687 | 6.80 ± 0.75 | 3.30 ± 0.20 | 0.547 ± 0.078 | 0.011 | TTV | (Hadden & Lithwick 2017) |
| Kepler-23 c | 10.740 | 7.81 ± 1.26 | 3.005 ± 0.074 | 0.72 ± 0.12 | 0.012 | TTV | (Leleu et al. 2023) |
| Kepler-305 d | 16.739 | 6.20 ± 1.55 | 2.76 ± 0.12 | 0.65 ± 0.17 | 0.019 | TTV | (Leleu et al. 2023) |
| K2-136 c | 17.307 | 18.10 ± 1.85 | 3.00 ± 0.13 | 1.68 ± 0.20 | 0.022 | RV* | (Mayo et al. 2023) |
| Kepler-57 b | 5.720 | 25.06 ± 5.03 | 3.135 ± 0.089 | 2.18 ± 0.45 | 0.028 | TTV | (Leleu et al. 2023) |
| Kepler-36 c | 16.233 | 7.13 ± 0.18 | 3.679 ± 0.093 | 0.488 ± 0.022 | 0.031 | TTV | (Vissapragada et al. 2020) |
| TOI-125 c | 9.151 | 6.63 ± 0.99 | 2.759 ± 0.100 | 0.70 ± 0.11 | 0.034 | RV | (Nielsen et al. 2020) |
| K2-32 d | 31.717 | 6.70 ± 2.50 | 3.48 ± 0.12 | 0.50 ± 0.19 | 0.035 | RV | (Lillo-Box et al. 2020) |
| K2-32 c | 20.661 | 8.10 ± 2.40 | 3.13 ± 0.11 | 0.70 ± 0.21 | 0.035 | RV | (Lillo-Box et al. 2020) |
| Kepler-33 e | 31.784 | 5.50 ± 1.15 | 3.50 ± 0.75 | 0.41 ± 0.15 | 0.040 | TTV | (Hadden & Lithwick 2017) |
| Kepler-549 b | 42.950 | 11.00 ± 3.70 | 3.10 ± 0.40 | 0.97 ± 0.38 | 0.078 | TTV | (Hadden & Lithwick 2017) |
| Kepler-89 c | 10.424 | 7.80 ± 2.70 | 3.80 ± 0.65 | 0.51 ± 0.22 | 0.143 | TTV | (Hadden & Lithwick 2017) |
| WASP-47 d | 9.031 | 14.20 ± 1.30 | 3.567 ± 0.045 | 1.018 ± 0.095 | 0.171 | RV* | (Bryant & Bayliss 2022) |
| TOI-125 d | 19.980 | 13.60 ± 1.20 | 2.93 ± 0.17 | 1.31 ± 0.16 | 0.183 | RV | (Nielsen et al. 2020) |
| EPIC 249893012 c | 15.624 | 14.67 ± 1.86 | 3.67 ± 0.15 | 1.01 ± 0.14 | 0.288 | RV | (Hidalgo et al. 2020) |
| EPIC 249893012 d | 35.747 | 10.18 ± 2.44 | 3.94 ± 0.12 | 0.63 ± 0.15 | 0.288 | RV | (Hidalgo et al. 2020) |
| HD 136352 c | 27.592 | 11.24 ± 0.64 | 2.916 ± 0.074 | 1.088 ± 0.074 | 0.383 | RV | (Delrez et al. 2021) |
| HD 73583 b | 6.398 | 10.20 ± 3.25 | 2.790 ± 0.100 | 1.05 ± 0.34 | 0.951 | RV* | (Barragán et al. 2022) |
| K2-138 g | 41.968 | 4.32 ± 4.14 | 3.01 ± 0.28 | 0.40 ± 0.39 | 1.290 | RV | (Lopez et al. 2019) |
| EPIC 220674823 c | 13.340 | 8.90 ± 2.40 | 2.836 ± 0.079 | 0.90 ± 0.25 | 21.350 | RV | (Bonomo et al. 2023) |
| TOI-431 d | 12.461 | 9.90 ± 1.51 | 3.290 ± 0.090 | 0.80 ± 0.13 | 23.428 | RV | (Osborn et al. 2021) |
| HD 3167 c | 29.845 | 11.13 ± 0.76 | 3.00 ± 0.33 | 1.03 ± 0.18 | 29.101 | RV | (Bonomo et al. 2023) |
| HD 183579 b | 17.471 | 19.70 ± 3.95 | 3.55 ± 0.14 | 1.42 ± 0.30 | - | RV | (Palatnick et al. 2021) |
| TOI-220 b | 10.695 | 13.80 ± 1.00 | 3.03 ± 0.15 | 1.26 ± 0.13 | - | RV | (Hoyer et al. 2021) |
| TOI-1052 b | 9.140 | 16.90 ± 1.70 | 2.87 ± 0.27 | 1.68 ± 0.29 | - | RV | (Armstrong et al. 2023) |
| TOI-1231 b | 24.246 | 15.40 ± 3.30 | 3.65 ± 0.15 | 1.07 ± 0.24 | - | RV* | (Burt et al. 2021) |
Notes. RV planets with no marker have either been only observed by HARPS, or by simultaneously (i.e. overlapping points withing few tens of days) by HARPS and another telescope. K2-136 was first observed by HARPS-N then ESPRESSO, WASP-47 was first observed by Coralie, then by ESPRESSO, HD 73583 was first observed by Coralie, then by HARPS, and TOI-1231 was first observed by PFS.
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